Celestial Atlas
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Page last updated Apr 29, 2014
WORKING: Add basic pix, tags

NGC 800 = (PGC 7740)
Discovered (Oct 9, 1885) by
Lewis Swift (2-17)
A 13th-magnitude spiral galaxy (type SA(rs)c) in Cetus (RA 02 02 11.8, Dec -00 07 51)
The second Index Catalog lists a corrected 1860 RA (per Howe) of 01 55 92. Paired with NGC 799. Based on a recessional velocity of 5965 km/sec, NGC 800 is about 265 million light years away. Given that and its apparent size of 1.05 by 0.7 arcmins, it is about 80 thousand light years across.
SDSS image of spiral galaxy NGC 800
Above, a 2.4 arcmin wide closeup of NGC 800
Below, a 12 arcmin wide region centered on its companion, NGC 799
SDSS image of region near spiral galaxies NGC 799 and 800

NGC 801 (= PGC 7847)
Discovered (Sep 20, 1885) by
Lewis Swift (2-18)
A 13th-magnitude spiral galaxy (type Sc) in Andromeda (RA 02 03 44.9, Dec +38 15 34)
Apparent size 3.1 by 0.7 arcmin.
DSS image of spiral galaxy NGC 801
Above, a 3.6 arcmin wide closeup of NGC 801
Below, a 12 arcmin wide region centered on the galaxy
DSS image of region near spiral galaxy NGC 801

NGC 802 (= PGC 7505)
Discovered (Nov 2, 1834) by
John Herschel (GC 482, JH 2457)
A 13th-magnitude lenticular galaxy (type SB0/a) in Hydrus (RA 01 59 06.1, Dec -67 52 13)
Apparent size 0.9 by 0.6 arcmin.

NGC 803 (= PGC 7849)
Discovered (Oct 15, 1784) by
William Herschel (GC 483, JH 190, WH III 208)
A 13th-magnitude spiral galaxy (type Sc) in Aries (RA 02 03 44.8, Dec +16 01 52)
Apparent size 3.0 by 1.3 arcmin.
SDSS image of spiral galaxy NGC 803
Above, a 3.6 arcmin wide closeup of NGC 803
Below, a 12 arcmin wide region centered on the galaxy
SDSS image of region near spiral galaxy NGC 803

NGC 804 (=
IC 1773 = PGC 7873)
Discovered (Sep 7, 1885) by Lewis Swift (2-19) (and later listed as NGC 804)
Discovered (Dec 24, 1897) by Guillaume Bigourdan (and later listed as IC 1773)
A 14th-magnitude lenticular galaxy (type S0) in Triangulum (RA 02 04 02.2, Dec +30 49 57)
Apparent size 1.4 by 0.3 arcmin.

NGC 805 (= PGC 7899)
Discovered (Sep 26, 1864) by
Heinrich d'Arrest (GC 5212)
A 14th-magnitude lenticular galaxy (type SB0) in Triangulum (RA 02 04 29.5, Dec +28 48 46)
Apparent size 1.1 by 0.7 arcmin.

NGC 806 (= PGC 7835 + PGC 3100716)
Discovered (Nov 1, 1886) by
Lewis Swift (5-19)
A pair of interacting galaxies in Cetus
PGC 7835 = A 14th-magnitude spiral galaxy (type Sc) at RA 02 03 31.2, Dec -09 55 58
PGC 3100716 = A 15th-magnitude spiral galaxy (type S) at RA 02 03 32.4, Dec -09 55 46
Apparent size of PGC 7835 = 1.2 by 0.4 arcmin; of PGC 3100716 = 0.4 by 0.2 arcmin. There is little doubt that the two objects are either colliding galaxies, or the result of a collision.
SDSS image of colliding galaxy pair NGC 806, showing labels for the individual components, PGC 7835 and PGC 3100716
Above, a 2.4 arcmin wide closeup of NGC 806, showing labels for the individual components
Below, a 12 arcmin wide region centered on the pair
SDSS image of region near colliding galaxy pair NGC 806

NGC 807 (= PGC 7934)
Discovered (Sep 11, 1784) by
William Herschel (GC 484, JH 191, WH III 151)
A 13th-magnitude elliptical galaxy (type E3) in Triangulum (RA 02 04 55.5, Dec +28 59 16)
Apparent size 1.8 by 1.3 arcmin.

NGC 808 (= PGC 7865)
Discovered (Oct 14, 1830) by
John Herschel (GC 485, JH 192 = JH 2458)
A 14th-magnitude spiral galaxy (type SBbc) in Cetus (RA 02 03 56.5, Dec -23 18 44)
Apparent size 1.2 by 0.6 arcmin.
DSS image of spiral galaxy NGC 808
Above, a 2.4 arcmin wide closeup of NGC 808
Below, a 12 arcmin wide region centered on the galaxy
DSS image of region near spiral galaxy NGC 808

NGC 809 (= PGC 7889)
Discovered (Nov 1, 1886) by
Lewis Swift (5-20)
A 14th-magnitude lenticular galaxy (type S0) in Cetus (RA 02 04 18.9, Dec -08 44 06)
The second Index Catalog lists a corrected RA (per Howe) of 01 57 25. Apparent size 1.2 by 0.9 arcmin.

NGC 810 (= PGC 7965)
Discovered (Dec 11, 1871) by
Édouard Stephan (3-5, GC 5213)
A 14th-magnitude elliptical galaxy (type E2 pec) in Aries (RA 02 05 28.6, Dec +13 15 04)
Apparent size 1.7 by 1.3 arcmin. NGC 810 appears to have a double nucleus, implying that it may be a double system in the last stages of a merger. It also has a much smaller apparent companion (PGC 3126708, a 16th-magnitude elliptical galaxy (type E5?) of apparent size 0.2 by 0.1 arcmin) 0.8s east of the larger galaxy's double nucleus. The recessional velocity of NGC 810 is 7795 km/sec, and PGC 3126708's recessional velocity is 7420 km/sec, so this may well be a triple system.
SDSS image of elliptical galaxy NGC 810 and its possible companion, elliptical galaxy PGC 3126708
Above, a 2.4 arcmin wide closeup of NGC 810 and its possible companion
Below, a 12 arcmin wide region centered on the galaxy
SDSS image of region near elliptical galaxy NGC 810

NGC 811 (= PGC 7870)
Discovered (1886) by
Francis Leavenworth
A 14th-magnitude spiral galaxy (type S) in Cetus (RA 02 04 00.0, Dec -09 06 21)
Per Dreyer, NGC 811 (= Leavenworth list II (#324), 1860 RA 01 57 55, NPD 99 46.7) is "extremely faint, extremely small, round (questionable nebulosity), with a star 1' to the south". The position precesses to RA 02 04 49.5, Dec -09 06 20, but there is nothing there. This has led to considerable confusion about the identity of the object. Most references associate NGC 811 with PGC 7905, but per Corwin the correct identification is almost certainly PGC 7870, which lies almost exactly 50s to the west (suggesting a carrying error in the reduction), and exactly matches the description, down to the star 1 arcmin to the south. Based on a recessional velocity of 14665 km/sec, a straightforward calculation indicates that NGC 811 is about 685 million light years away. However, for objects at such distances we should take into account the Universal expansion during the time it took their light to reach us. Doing that shows that the galaxy was about 635 million light years away at the time the light by which we see it was emitted, about 650 million years ago (the difference between the two numbers being due to the expansion of the intervening space during the light-travel time). Given that and its apparent size of 0.6 by 0.55 arcmin, NGC 811 is about 110 thousand light years across. (Note: Listed in NED as 6dFJ0204000-090622.)
SDSS image of spiral galaxy NGC 811
Above, a 2.4 arcmin wide closeup of NGC 811
Below, a 12 arcmin wide region centered on the galaxy
SDSS image of region near spiral galaxy NGC 811
Below, a 20 arcmin wide region centered between Dreyer's position and the actual position of NGC 811
SDSS image of region between Dreyer's position for NGC 811 (shown by a box) and the actual position of the galaxy

PGC 7905 (not =
NGC 811)
Not an NGC object, but listed here because usually (erroneously) identified as NGC 811
A 15th-magnitude spiral galaxy (type SB(s)d?) in Cetus (RA 02 04 34.8, Dec -10 06 31)
As noted at the entry for NGC 811, PGC 7905 is usually identified as that object. However, that identification is suspect on two counts. First, although errors in declination do occur in the original NGC, they are far less common than errors in right ascension; so the 50s of time error for PGC 7870 is not as surprising as the 70 arcmin error in declination that would be required for PGC 7905 to be Leavenworth's object. Second, the original observation stated that there was a star just south of the galaxy, as is true for PGC 7870 but not for PGC 7905. Still, since PGC 7905 is so commonly misidentified as NGC 811, it seems appropriate to discuss it here. Based on a recessional velocity of 1925 km/sec, PGC 7905 is about 90 million light years away. Given that and its apparent size of 1.0 by 0.5 arcmin, it is about 25 thousand light years across.
SDSS image of spiral galaxy PGC 7905, which is usually misidentified as NGC 811
Above, a 2.4 arcmin wide closeup of PGC 7905
Below, a 12 arcmin wide region centered on the galaxy
SDSS image of region near spiral galaxy PGC 7905, which is usually misidentified as NGC 811

NGC 812 (= PGC 8066)
Discovered (Dec 11, 1876) by
Édouard Stephan (8-3, GC 5214)
An 11th-magnitude spiral galaxy (type Sbc) in Andromeda (RA 02 06 51.7, Dec +44 34 21)
Apparent size 2.2 by 0.8 arcmin.
DSS image of spiral galaxy NGC 812
Above, a 2.4 arcmin wide closeup of NGC 812
Below, a 12 arcmin wide region centered on the galaxy
DSS image of region near spiral galaxy NGC 812

NGC 813 (= PGC 7692)
Discovered (Nov 24, 1834) by
John Herschel (GC 486, JH 2459)
A 13th-magnitude lenticular galaxy (type SB0/a) in Hydrus (RA 02 01 36.1, Dec -68 26 21)
Apparent size 1.3 by 0.9 arcmin.

NGC 814 (= PGC 8319)
Discovered (Jan 6, 1886) by
Ormond Stone
A 14th-magnitude lenticular galaxy (type SB0° pec?) in Cetus (RA 02 10 37.6, Dec -15 46 24)
Per Dreyer, NGC 814 (= Ormond Stone list I (#47), 1860 RA 01 59 35, NPD 106 25.7) is "extremely faint, small, round, gradually brighter middle". The position precesses to RA 02 06 17.7, Dec -15 45 29, but there is nothing there. As a result NGC 814 and 815, which was found by Stone on the same night and suffered the same error in its recorded position, were considered lost or most recently misidentified with a pair of galaxies (PGC 7799 and 7798, respectively) that have the same difference in their relative position (4 arcmin north and south of each other) as NGC 814 and 815, but lie about 4m west and 70 arcmin north of Stone's positions. Such errors in right ascension, although unfortunate, are not unusual in the NGC, particularly for some observers (such as Stone); and in fact the correct identification of the objects (PGC 8319 and 906183, as shown in the entries here) involves a 4m 20s error in right ascension in the opposite direction (that is, to the east of Stone's position). Large errors in North Polar Declination are not as common, so the fact that the current candidates for NGC 814 and 815 lie only 1 arcmin south of Stone's position instead of the 70 arcmin north for the prior candidates would make them seem a more reasonable solution even without any additional information. However, we needn't try to decide which galaxies are more likely to be what Stone observed merely on the basis of preference, as (per Corwin) Stone made a sketch of the area with an "unmistakable" starfield, making the current identification certain (for novices, this means that the positions of the stars and nebulae in the sky match the sketch only if the nebulae are PGC 8319 and 906183). As a result most major catalogues (such as NED and LEDA) have switched to the new identification, but because of the historical confusion associated with the identification of NGC 814 and 815, other resources (such as Wikisky) still show the older identification, and odds are that at least some confusion will persist for a long time to come; so the objects previously misidentified as these NGC entries are also covered here, immediately following the correct entries. Based on a recessional velocity of 1615 km/sec, PGC 8319 (= NGC 814) is about 75 million light years away. Given that and its apparent size of 1.4 by 0.6 arcmin, it is about 30 thousand light years across.
DSS image of lenticular galaxy PGC 8319, now identified as NGC 814
Above, a 2.4 arcmin wide closeup of NGC 814
Below, a 12 arcmin wide region centered between NGC 814 and 815
DSS image of region near lenticular galaxy PGC 8319, now identified as NGC 814, and spiral galaxy PGC 906183, now identified as NGC 815
Below, a 12 arcmin wide region centered between Ormond Stone's positions for NGC 814 and 815
DSS image of the region near Ormond Stone's positions for NGC 814 and 815, shown by boxes for historical purposes
Below, a 2 degree wide region with circles showing Ormond Stone's positions for NGC 814 and 815, the position of the erroneous candidates PGC 7798 and 7799, and the position of the correct NGC objects. The correct positions are at almost the same declination as Stone's, and even without the certainty provided by his sketch of the region, would make the new identification seem more likely.
DSS image with circles showing Ormond Stone's positions for NGC 814 and 815, the position of the erroneous candidates PGC 7798 and 7799, and the position of the correct NGC objects

NGC 815 (= PGC 906183)
Discovered (Jan 6, 1886) by
Ormond Stone
A 16th-magnitude pair of compact galaxies (type C + C) in Cetus (RA 02 10 39.4, Dec -15 48 46)
Per Dreyer, NGC 815 (= Ormond Stone list I (#48), 1860 RA 01 59 35, NPD 106 29.7) is "extremely faint, very small, round, gradually brighter middle". The position precesses to RA 02 06 17.5, Dec -15 49 29, but there is nothing there, and for a long time the entry was "lost" or misidentified (most recently as PGC 7798). However, as noted in the entry for NGC 814 (which see for a detailed discussion), Stone made a sketch that unmistakably confirms PGC 9318 and PGC 906183 as the correct identification of NGC 814 and 815. Based on a recessional velocity of 16080 km/sec, a straightforward calculation indicates that NGC 815 is about 750 million light years away. However, for objects at such distances we should take into account the Universal expansion during the time it took their light to reach us. Doing that shows that the galaxy was about 695 million light years away at the time the light by which we see it was emitted, about 715 million years ago (the difference between the two numbers being due to the expansion of the intervening space during the light-travel time). Given that and its apparent size of 0.45 by 0.2 arcmin, the pair spans about 90 thousand light years. (Note: NGC 815 is listed in NED as APMUKS(BJ) B020815.78-160253.1, with the same position that LEDA lists for PGC 906183.)
DSS image of compact galaxy pair PGC 906183, now identified as NGC 815
Above, a 2.4 arcmin wide closeup of NGC 815; see NGC 814 for wide-field images

PGC 7799 (not =
NGC 814)
Not an NGC object, but listed here because often misidentified as NGC 814
A 15th-magnitude spiral galaxy (type LEDA SABb/NED SB(s)d) in Cetus (RA 02 02 56.5, Dec -14 36 32)
As discussed at the entry for NGC 814, PGC 7799 is a recent but erroneous candidate for NGC 814. Since it is about 4m west and nearly 70' north of Stone's position it hardly seems an ideal candidate, but when objects are "lost" misidentifications are common, and since PGC 7799 and 7798 (which was commonly misidentified as NGC 815) are about the same 4 arcmin apart as NGC 814 and 815, the misidentification is understandable, even if unfortunate. Based on a recessional velocity of 3735 km/sec, PGC 7799 is about 175 million light years away. Given that and its apparent size of 0.8 by 0.5 arcmin, it is about 40 thousand light years across.
DSS image of spiral galaxy PGC 7799, often misidentified as NGC 814
Above, a 2.4 arcmin wide closeup of PGC 7799
Below, a 12 arcmin wide region centered between PGC 7799 and 7798
DSS image of spiral galaxies PGC 7799, often misidentified as NGC 814, and PGC 7798, often misidentified as NGC 815

PGC 7798 (not =
NGC 815)
Not an NGC object, but listed here because often misidentified as NGC 815
A 15th-magnitude spiral galaxy (type SB(s)m?) in Cetus (RA 02 02 54.2, Dec -14 40 23)
As discussed at the entry for NGC 814, PGC 7798 is a recent but erroneous candidate for NGC 815. Since it is about 4m west and nearly 70' north of Stone's position it hardly seems an ideal candidate, but when objects are "lost" misidentifications are common, and since PGC 7798 and 7799 (which was commonly misidentified as NGC 814) are about the same 4 arcmin apart as NGC 815 and 814, the misidentification is understandable, even if unfortunate. PGC 7798 has an apparent size of 1.0 by 0.5 arcmin, but apparently nothing else is available, so its distance and size are unknown.
DSS image of spiral galaxy PGC 7798, often misidentified as NGC 815
Above, a 2.4 arcmin wide closeup of PGC 7798; see PGC 7799 for a wide-field image

NGC 816 (= PGC 8152)
Discovered (Sep 15, 1871) by
Édouard Stephan (6-1, GC 5215)
A 14th-magnitude compact galaxy (type C) in Triangulum (RA 02 08 08.8, Dec +29 15 23)
Apparent size 0.4 by 0.4 arcmin.

NGC 817 (= PGC 8109)
Discovered (Sep 2, 1886) by
Lewis Swift (4-7)
A 13th-magnitude spiral galaxy (type S?) in Aries (RA 02 07 33.6, Dec +17 12 07)
The first Index Catalog corrects (per Bigourdan) the seconds of RA to 44. Apparent size 0.7 by 0.3 arcmin.
SDSS image of spiral galaxy NGC 817
Above, a 2.4 arcmin wide closeup of NGC 817
Below, a 12 arcmin wide region centered on the galaxy
SDSS image of region near spiral galaxy NGC 817

NGC 818 (= PGC 8185)
Discovered (Oct 18, 1786) by
William Herschel (GC 488, JH 194, WH II 604)
A 13th-magnitude spiral galaxy (type SBbc) in Andromeda (RA 02 08 44.4, Dec +38 46 38)
Apparent size 2.9 by 1.2 arcmin.
DSS image of spiral galaxy NGC 818
Above, a 3 arcmin wide closeup of NGC 818
Below, a 12 arcmin wide region centered on the galaxy
DSS image of region near spiral galaxy NGC 818

NGC 819 (= PGC 8174)
Discovered (Sep 20, 1865) by
Heinrich d'Arrest (GC 5216)
Also observed (Sep 15, 1871) by Édouard Stephan
A 14th-magnitude spiral galaxy (type S?) in Triangulum (RA 02 08 34.5, Dec +29 14 05)
Apparent size 0.6 by 0.4 arcmin.
SDSS image of spiral galaxy NGC 819
Above, a 2.4 arcmin wide closeup of NGC 819
Below, a 12 arcmin wide region centered on the galaxy
SDSS image of region near spiral galaxy NGC 819

NGC 820 (= PGC 8165)
Discovered (Sep 7, 1828) by
John Herschel (GC 489, JH 195)
A 13th-magnitude spiral galaxy (type Sb) in Aries (RA 02 08 24.9, Dec +14 20 59)
Apparent size 1.4 by 0.8 arcmin.
SDSS image of spiral galaxy NGC 820
Above, a 2.4 arcmin wide closeup of NGC 820
Below, a 12 arcmin wide region centered on the galaxy
SDSS image of region near spiral galaxy NGC 820

NGC 821 (= PGC 8160)
Discovered (Sep 4, 1786) by
William Herschel (GC 487, JH 193, WH I 152)
An 11th-magnitude elliptical galaxy (type E6) in Aries (RA 02 08 21.0, Dec +10 59 39)
Apparent size 2.4 by 1.7 arcmin.

NGC 822 (= PGC 8055)
Discovered (Sep 5, 1834) by
John Herschel (GC 490, JH 2461)
A 13th-magnitude elliptical galaxy (type E5) in Phoenix (RA 02 06 39.2, Dec -41 09 25)
Apparent size 1.1 by 0.6 arcmin.

NGC 823 (=
IC 1782 = PGC 8093)
Discovered (Oct 14, 1830) by John Herschel (GC 491, JH 196 = JH 2460) (and later listed as NGC 823)
Discovered (Oct 8, 1896) by Lewis Swift (and later listed as IC 1782)
A 13th-magnitude lenticular galaxy (type E/S0) in Fornax (RA 02 07 20.0, Dec -25 26 30)
Apparent size 1.7 by 1.3 arcmin.

NGC 824 (= PGC 8068)
Discovered (Nov 29, 1837) by
John Herschel (GC 492, JH 2462)
A 13th-magnitude spiral galaxy (type SBbc) in Fornax (RA 02 06 53.2, Dec -36 27 12)
Apparent size 1.4 by 1.2 arcmin.
DSS image of spiral galaxy NGC 824
Above, a 2.4 arcmin wide closeup of NGC 824
Below, a 12 arcmin wide region centered on the galaxy
DSS image of region near spiral galaxy NGC 824

NGC 825 (= PGC 8173)
Discovered (Nov 18, 1863) by
Albert Marth (53, GC 5217)
A 13th-magnitude spiral galaxy (type Sa) in Cetus (RA 02 08 32.4, Dec +06 19 24)
Apparent size 2.0 by 0.5 arcmin.
SDSS image of spiral galaxy NGC 825
Above, a 2.4 arcmin wide closeup of NGC 825
Below, a 12 arcmin wide region centered on the galaxy, also showing IC 208
SDSS image of region near spiral galaxy NGC 825, also showing spiral galaxy IC 208

NGC 826 (= PGC 8230)
Discovered (Sep 18, 1871) by
Édouard Stephan
A pair of galaxies in Triangulum
PGC 8230 = A 14th-magnitude lenticular galaxy (type E/S0?) at RA 02 09 25.1, Dec +30 44 22
"NGC 826-2" = A 15th-magnitude spiral galaxy (type S) at RA 02 09 24.8, Dec +30 44 37
Per Dreyer, NGC 826 (= GC 5218 = Stephan list VI (#3), 1860 RA 02 01 18, NPD 59 55.5) is "extremely faint, small, round, little brighter middle". The position precesses to RA 02 09 25.4, Dec +30 44 27, essentially dead-on PGC 8230, so the identification is certain. However, its current-day galaxy type is uncertain, being listed as S? in one reference, and E4 in another. The images below show some evidence of dusty obscuration of or by PGC 8230's apparent companion ("NGC 826-2"), but no evidence of spiral structure in the brighter galaxy; hence my decision to list its type as intermediate (that is, lenticular). Based on a recessional velocity of 4865 km/sec, NGC 826 is about 225 million light years away. Given that and its apparent size of 0.75 by 0.45 arcmin, it is about 50 thousand light years across. As far as its companion is concerned, it cannot have made any significant contribution to what Stephan saw, so as far as the NGC listing is concerned its presence is merely an accident, and PGC 8230 is NGC 826; but as the 'name' of the companion shows, it is treated as one component of a multiple galaxy. In some cases that would be mentioned in discussions of the larger galaxy; but every reference to PGC 8230 lists it as a single object, so its companion must be treated as a separate entity. However, other than its apparent size of 0.3 by 0.1 arcmin and the information in the single line above, I can find nothing about "NGC 826-2". There is no mention of it or any other object near its position (save for NGC 826 itself) in any catalog, and its appellation as NGC 826-2 appears to have been created only for the purpose of discussing it in entries such as this one. It isn't even clear whether it is actually a physical companion of the larger galaxy, or merely an optical double. There is some dusty obscuration surrounding the region it occupies, which could be silhouetting of clouds of dust in the smaller galaxy against the background of the larger galaxy, or vice-versa. The shape of the obscuration suggests that the smaller galaxy is a foreground object, but the faintness of its nearer arm (that is, the one closer to the nucleus of NGC 826) suggests that it is a background object. So in addition to almost nothing being known about the smaller galaxy's physical characteristics, nothing is known about its relationship to its larger "companion".
SDSS image of lenticular galaxy NGC 826 and its apparent companion, usually referred to (if referred to at all) as 'NGC 826-2'
Above, a 2.4 arcmin wide closeup of NGC 826 and its apparent companion
Below, a 12 arcmin wide region centered on the pair
SDSS image of region near lenticular galaxy NGC 826

NGC 827 (= PGC 8196)
Discovered (Nov 7, 1784) by
William Herschel (GC 493 = JH 198 = WH III 227)
Also observed (Oct 9, 1884) by Lewis Swift
A 13th-magnitude spiral galaxy (type Sbc) in Cetus (RA 02 08 56.3, Dec +07 58 18)
Apparent size 2.0 by 0.6 arcmin.
DSS image of spiral galaxy NGC 827
Above, a 2.4 arcmin wide closeup of NGC 827
Below, a 12 arcmin wide region centered on the galaxy
DSS image of region near spiral galaxy NGC 827

NGC 828 (= PC 8283)
Discovered (Oct 18, 1786) by
William Herschel (GC 494, JH 197, WH II 605)
A 12th-magnitude spiral galaxy (type Sa pec) in Andromeda (RA 02 10 09.5, Dec +39 11 28)
Apparent size 2.5 by 1.6 arcmin.
DSS image of spiral galaxy NGC 828
Above, a 3 arcmin wide closeup of NGC 828
Below, a 12 arcmin wide region centered on the galaxy
DSS image of region near spiral galaxy NGC 828

NGC 829 (= PGC 8182)
Discovered (Sep 23, 1865) by
Heinrich d'Arrest (GC 5219)
A 14th-magnitude spiral galaxy (type Sc) in Cetus (RA 02 08 42.2, Dec -07 47 25)
Apparent size 1.1 by 0.6 arcmin.
SDSS image of spiral galaxy NGC 829
Above, a 3 arcmin wide closeup of NGC 829
Below, a 12 arcmin wide region centered on the galaxy, also showing NGC 830
SDSS image of region near spiral galaxy NGC 829, also showing lenticular galaxy NGC 830

NGC 830 (= PGC 8201)
Discovered (Sep 23, 1865) by
Heinrich d'Arrest (GC 5220)
A 13th-magnitude lenticular galaxy (type E/S0) in Cetus (RA 02 08 58.7, Dec -07 46 03)
Apparent size 1.4 by 0.9 arcmin. (for now, see NGC 829 for a wide-field image)

NGC 831 (= PGC 8241)
Discovered (Nov 18, 1863) by
Albert Marth (54, GC 5221)
A 15th-magnitude spiral galaxy (type S?) in Cetus (RA 02 09 34.5, Dec +06 05 48)
Apparent size 0.4 by 0.3 arcmin.
SDSS image of spiral galaxy NGC 831
Above, a 2.4 arcmin wide closeup of NGC 831
Below, a 12 arcmin wide region centered on the galaxy
SDSS image of region near spiral galaxy NGC 831

NGC 832
Recorded (Sep 17, 1865) by
Heinrich d'Arrest
Perhaps a pair of stars in Triangulum (RA 02 11 00.7, Dec +35 32 30)
Per Dreyer, NGC 832 (=GC 5222 = d'Arrest, 1860 RA 02 02 17, NPD 55 07.6) is "faint, very small, 9th or 10th magnitude star to the southwest". The position precesses to RA 02 10 36.5, Dec +35 32 14, but there is nothing there. The tentative identification of the pair of stars at the location listed above as NGC 832 is based (per Corwin) on the fact that there is a 10th-magnitude star to the southeast of d'Arrest's recorded position, and that star is to the southwest of the pair of stars 24s to the east of the recorded position. In other words, there is a possibility that the pair of stars is what d'Arrest observed (they could easily look like a very small nebula under less than ideal observing conditions), and he misrecorded the direction of the brighter star, as well as the position of the 'object' he observed. Similar errors are not uncommon in the NGC, so if forced to choose something as NGC 832 the pair of stars is as good a choice as any. However, it is also possible that the correct designation for this entry is "lost or nonexistent".
DSS image of the region between d'Arrest's position for NGC 832 (shown by a box) and the pair of stars tentatively identified as what he actually observed
Above, a 12 arcmin wide region showing d'Arrest's position for NGC 832 (shown by a box) and its tentative identification as the pair of stars to the east of his position. The 10th-magnitude star at the heart of Corwin's argument is circled.

NGC 833 (= PGC 8225, and with
NGC 835, 838 and 839 = Arp 318 = HCG 16)
Discovered (Nov 28, 1785) by William Herschel (GC 495, JH 99 = JH 2463, WH II 482)
A 13th-magnitude spiral galaxy (type Sa pec) in Cetus (RA 02 09 20.8, Dec -10 07 58)
Apparent size 1.5 by 0.7 arcmin.
SDSS image of spiral galaxy NGC 833 and part of spiral galaxy NGC 835, which are part of Arp 318, also known as Hickson Compact Group 16
Above, a 2.4 arcmin wide closeup of NGC 833 and part of NGC 835
Below, a 12 arcmin wide region centered on the galaxy, also showing NGC 835, 838 and 839
SDSS image of region near spiral galaxy NGC 833, also showing spiral galaxy 835 and lenticular galaxies NGC 838 and 839, which are called Arp 318, also known as Hickson Compact Group 16, overlaid on a DSS background to fill in missing areas
Below, a 6 arcmin wide region centered on Arp 318, which consists of NGC 833, 835, 838 and 839
SDSS image of region near spiral galaxies NGC 833 and 835, and lenticular galaxies NGC 838 and 839, collectively also known as Arp 318 or Hickson Compact Group 16, overlaid on a DSS background to fill in missing regions

NGC 834 (= PGC 8352)
Discovered (Sep 21, 1786) by
William Herschel
A 13th-magnitude spiral galaxy (type Sbc) in Andromeda (RA 02 11 01.2, Dec +37 39 58)
Per Dreyer, NGC 834 (= GC 496 = WH III 567, 1860 RA 02 02 32, NPD 53 00.7) is "very faint, small, a little extended". The position precesses to RA 02 10 57.2, Dec +37 39 06, less than an arcmin southwest of the galaxy, so the identification is certain. Apparent size 1.1 by 0.5 arcmin.
DSS image of spiral galaxy NGC 834
Above, a 2.4 arcmin wide closeup of NGC 834
Below, a 12 arcmin wide region centered on the galaxy
DSS image of region near spiral galaxy NGC 834

NGC 835 (= PGC 8228, and with
NGC 833, 838 and 839 = Arp 318 = HCG 16)
Discovered (Nov 28, 1785) by William Herschel (GC 497, JH 200 = JH 2464, WH II 483)
A 12th-magnitude spiral galaxy (type SBab pec) in Cetus (RA 02 09 24.6, Dec -10 08 07)
Apparent size 1.3 by 1.1 arcmin.
SDSS image of spiral galaxy NGC 835 and part of spiral galaxy NGC 833, which are part of Arp 318, also known as Hickson Compact Group 16
Above, a 3 arcmin wide closeup of NGC 835, also showing part of NGC 833
Below, a 12 arcmin wide region centered on the galaxy, also showing NGC 833, 838 and 839
SDSS image of region near spiral galaxy NGC 835, also showing spiral galaxy NGC 833 and lenticular galaxies NGC 838 and 839, which are called Arp 318, also known as Hickson Compact Group 16, overlaid on a DSS background to fill in missing areas
Below, a 6 arcmin wide region centered on Arp 318, which consists of NGC 833, 835, 838 and 839
SDSS image of region near spiral galaxies NGC 833 and 835, and lenticular galaxies NGC 838 and 839, collectively also known as Arp 318 or Hickson Compact Group 16, overlaid on a DSS background to fill in missing regions

NGC 836 (= PGC 8304)
Discovered (1886) by
Frank Muller (II-325)
A 13th-magnitude lenticular galaxy (type S0/a) in Cetus (RA 02 10 24.8, Dec -22 03 18)
The second Index Catalog lists a corrected 1860 RA (per Howe) of 02 03 55. Apparent size 1.2 by 0.9 arcmin.

NGC 837 (= PGC 8297)
Discovered (1886) by
Francis Leavenworth (II-326)
A 14th-magnitude spiral galaxy (type Sb) in Cetus (RA 02 10 16.1, Dec -22 25 53)
The second Index Catalog lists a corrected 1860 RA (per Howe) of 02 03 47. Apparent size 0.9 by 0.4 arcmin.
DSS image of spiral galaxy NGC 837
Above, a 2.4 arcmin wide closeup of NGC 837
Below, a 12 arcmin wide region centered on the galaxy
DSS image of region near spiral galaxy NGC 837

NGC 838 (= PGC 8250, and with
NGC 833, 835 and 839 = Arp 318 = HCG 16)
Discovered (Nov 28, 1785) by William Herschel (= GC 498, JH 201 = JH 2465, WH II 484)
A 13th-magnitude lenticular galaxy (type SA0(rs)a pec?) in Cetus (RA 02 09 38.4, Dec -10 08 45)
Apparent size 1.2 by 0.9 arcmin?
SDSS image of lenticular galaxy NGC 838, which is part of Arp 318, also known as Hickson Compact Group 16
Above, a 2.4 arcmin wide closeup of NGC 838
Below, a HST image of the galaxy (Image Credits Hubble Legacy Archive, post processing by Courtney Seligman)
HST image of lenticular galaxy NGC 838, which is part of Arp 318, also known as Hickson Compact Group 16
Below, a 12 arcmin wide region centered on the galaxy, also showing NGC 833, 835 and 839
SDSS image of region near lenticular galaxy NGC 838, also showing spiral galaxies NGC 833 and 835 and lenticular galaxy NGC 839, which are called Arp 318, also known as Hickson Compact Group 16, overlaid on a DSS background to fill in missing areas
Below, a 6 arcmin wide region centered on Arp 318, which consists of NGC 833, 835, 838 and 839
SDSS image of region near spiral galaxies NGC 833 and 835, and lenticular galaxies NGC 838 and 839, collectively also known as Arp 318 or Hickson Compact Group 16, overlaid on a DSS background to fill in missing regions

NGC 839 (= PGC 8254, and with
NGC 833, 835 and 838 = Arp 318 = HCG 16)
Discovered (Nov 28, 1785) by William Herschel (GC 499, JH 202 = JH 2466, WH II 485)
A 13th-magnitude lenticular galaxy (type S0) in Cetus (RA 02 09 42.9, Dec -10 11 00)
Apparent size 1.4 by 0.7 arcmin.
DSS image of lenticular galaxy NGC 839, which is part of Arp 318, also known as Hickson Compact Group 16
Above, a 2.4 arcmin wide closeup of NGC 839
Below, a 12 arcmin wide region centered on the galaxy, also showing NGC 833, 835 and 838
SDSS image of region near lenticular galaxy NGC 839, also showing spiral galaxies NGC 833 and 835 and lenticular galaxy NGC 838, which are called Arp 318, also known as Hickson Compact Group 16, overlaid on a DSS background to fill in missing areas
Below, a 6 arcmin wide region centered on Arp 318, which consists of NGC 833, 835, 838 and 839
SDSS image of region near spiral galaxies NGC 833 and 835, and lenticular galaxies NGC 838 and 839, collectively also known as Arp 318 or Hickson Compact Group 16, overlaid on a DSS background to fill in missing regions

NGC 840 (= PGC 8293)
Discovered (Sep 2, 1864) by
Albert Marth (55, GC 5223)
A 13th-magnitude spiral galaxy (type SBb) in Cetus (RA 02 10 16.1, Dec +07 50 45)
Apparent size 1.8 by 1.0 arcmin.
SDSS image of spiral galaxy NGC 840
Above, a 2.4 arcmin wide closeup of NGC 840
Below, a 12 arcmin wide region centered on the galaxy
SDSS image of region near spiral galaxy NGC 840

NGC 841 (= PGC 8372)
Discovered (Jan 17, 1787) by
William Herschel
Rediscovered (Nov 24, 1883) by Édouard Stephan
A 13th-magnitude spiral galaxy (type (R')SAB(s)ab) in Andromeda (RA 02 11 17.4, Dec +37 29 51)
Per Dreyer, NGC 841 (Stephan list XIII (#16), 1860 RA 02 02 52, NPD 53 10.0) is "pretty bright, very small, much brighter middle with a nucleus equal to a 13th or 14th magnitude star". The position precesses to RA 02 11 16.9, Dec +37 29 46, right on the galaxy, so the identification is certain. Although the identification is certain, the GC had an error that carried over to the NGC that confuses the discovery credits for NGC 841 and 845. William Herschel's WH III 604, which John Herschel thought was an earlier but incorrect observation of his JH 204 (= GC 501 = NGC 845), was actually an observation of NGC 841, and d'Arrest's supposed confirmation of those observations was also for NGC 841. So the NGC entry for NGC 841, "Stephan list XIII (#16)", should have read "WH III 604, d'Arrest, Stephan list XIII (#16)", and William Herschel was the original discoverer, not Stephan. However, when Stephan observed the region he used the GC (as most observers of the day would have) to compare his observations of the region to those of previous observers, and in that catalog the only suggestion that there might be a problem with the region is a note for GC 501 stating "C.H. (Caroline Herschel) and Auwers make the R.A. 1m less". If he'd thought about it, Stephan might have surmised that his observation of a nebula 1m to the west of GC 501 represented a duplication of a possible observation of the same nebula by William Herschel (as turned out to be the case), but since John Herschel thought the 1m difference was simply an error in previous observations of his JH 204, Stephan would have no reason to think otherwise. So he presumed he had found a new nebula, Dreyer agreed, and Stephan was given credit for discovering an object that William Herschel had already discovered. Stephan does deserve credit for rediscovering NGC 841, and being the first to notice that there were three nebulae in the region (now listed as NGC 834, 841 and 845). He just wasn't the first to observe any one of them. (Note: The history presented above is based on Corwin's notes; but since it is not presented in the same way, it did not seem appropriate to simply say "per Corwin".) Based on a recessional velocity of 4540 km/sec, NGC 841 is about 210 million light years away, in good agreement with redshift-independent distance estimates of 160 - 215 million light years. Given that and its apparent size of 1.8 by 1.0 arcmin, it is about 110 thousand light years across.
DSS image of spiral galaxy NGC 841
Above, a 2.4 arcmin wide closeup of NGC 841
Below, a 12 arcmin wide region centered on the galaxy
DSS image of region near spiral galaxy NGC 841

NGC 842 (= PGC 8258)
Discovered (Jan 8, 1831) by
John Herschel (GC 500, JH 203)
A 13th-magnitude lenticular galaxy (type S0) in Cetus (RA 02 09 50.7, Dec -07 45 45)
Per Dreyer, NGC 842 (= GC 500 = JH 203, 1860 RA 02 02 55, NPD 98 25.1) is "very faint, very small, round, pretty suddenly bright middle, the 3rd of 3", the others being NGC 829 and 830. The position precesses to RA 02 09 52.3, Dec -07 45 15, which is less than an arcmin northwest of the galaxy, so the identification is certain. Apparent size 1.6 by 0.8 arcmin.

NGC 843
Recorded (Sep 16, 1865) by
Heinrich d'Arrest (GC 5224)
Three stars in Triangulum (RA 02 11 08.2, Dec +32 05 54)
Per Dreyer, NGC 843 (= GC 5224 = d'Arrest, 1860 RA 02 02 56, NPD 58 34.0) is a "globular cluster, faint, small, round". The position precesses to RA 02 11 07.2, Dec +32 05 46, very close to a triple star that could look like a very small cluster under less than ideal observing conditions, so the identification is considered certain.

NGC 844 (= PGC 8291)
Discovered (Nov 18, 1863) by
Albert Marth
A 14th-magnitude compact galaxy (type C) in Cetus (RA 02 10 14.3, Dec +06 02 57)
Per Dreyer, NGC 844 (GC 5225 = Marth #56, 1860 RA 02 02 56, NPD 84 37) is "faint, small". The position precesses to RA 02 10 16.1, Dec +06 02 49, less than half an arcmin southeast of the galaxy, so the identification is certain. Apparent size 0.4 by 0.4 arcmin. (Note: A Wikisky search for NGC 844 or PGC 8291 shows an area just west of the galaxy, which is unlabeled.)

NGC 845 (= PGC 8438)
Not discovered by
William Herschel
Discovered (October 1828) by John Herschel
A 14th-magnitude spiral galaxy (type Sb) in Andromeda (RA 02 12 19.7, Dec +37 28 39)
Per Dreyer, NGC 845 (GC 501 = WH III 604 = JH 204, d'Arrest, 1860 RA 02 03 05, NPD 53 10.5) is "very faint, irregular figure, stellar". The position precesses to RA 02 11 30.0, Dec +37 29 15, which is about 3 arcmin east of NGC 841, and there is nothing else nearby, so it would appear that NGC 845 is a duplication of NGC 841, and in one sense that is true, due to an error in the GC that carried over to the NGC. Namely, William Herschel's WH III 604, which John Herschel thought was an earlier but incorrect observation of his JH 204 (= GC 501 = NGC 845), was actually an observation of NGC 841, and d'Arrest's supposed confirmation of those observations was also for NGC 841. For whatever reason, Dreyer used d'Arrest's position for the listing for NGC 845. If that position had been accurate, it would have been the same as for NGC 841, in which case Dreyer might not have bothered with another entry; but it was a bit off, so he concluded that GC 501 was a different object, and assigned it a different listing. This means that two corrections should be applied to the listing for NGC 845. First, "GC 501 = WH III 604 = JH 204, d'Arrest" should be replaced by "GC 501 = JH 204", which means that William Herschel was not the discoverer as usually stated, but his son John. Second, the position should be changed to that observed by John Herschel, since all the other observations refer to NGC 841, not NGC 845. The position listed by John Herschel for GC 501 is 1860 RA 02 03 56.7, NPD 53 10 55.5, which precesses to RA 02 12 22.2, Dec +37 28 40, which is right on the galaxy, and not only makes the identification certain, but proves that it is not a duplicate of NGC 841, after all. (Note: The history presented above is based on Corwin's notes; but since it is not presented in the same way, it did not seem appropriate to simply say "per Corwin".) Based on a recessional velocity of 4430 km/sec, NGC 845 is about 205 million light years away, in good agreement with a single redshift-independent distance estimate of 215 million light years. Given that and its apparent size of 1.7 by 0.4 arcmin, it is about 100 thousand light years across.
DSS image of spiral galaxy NGC 845
Above, a 2.4 arcmin wide closeup of NGC 845
Below, a 12 arcmin wide region centered on the galaxy
DSS image of region near spiral galaxy NGC 845

NGC 846 (=
NGC 847 = PGC 8430)
Discovered (Nov 22, 1876) by Édouard Stephan (and later listed as NGC 846)
Discovered (Nov 30, 1885) by Lewis Swift (and later listed as NGC 847)
A 12th-magnitude spiral galaxy (type SB(rs)ab) in Andromeda (RA 02 12 12.1, Dec +44 34 05)
Per Dreyer, NGC 846 (GC 5226 = Stephan list VIII (#4), 1860 RA 02 03 26, NPD 46 05.6) is "extremely faint, very small, round, gradually brighter middle". The position precesses to RA 02 12 12.7, Dec +44 34 05, right on the galaxy, so the identification is certain. Based on a recessional velocity of 5120 km/sec, NGC 846 is about 240 million light years away. Given that and its apparent size of 1.9 by 1.7 arcmin, it is about 130 thousand light years across.
DSS image of spiral galaxy NGC 846
Above, a 2.4 arcmin wide closeup of NGC 846
Below, a 12 arcmin wide region centered on the galaxy
DSS image of region near spiral galaxy NGC 846

NGC 847 (=
NGC 846 = PGC 8430)
Discovered (Nov 22, 1876) by Édouard Stephan (and later listed as NGC 846)
Discovered (Nov 30, 1885) by Lewis Swift (and later listed as NGC 847)
A 12th-magnitude spiral galaxy (type SBab) in Andromeda (RA 02 12 12.1, Dec +44 34 05)
Per Dreyer, NGC 847 (= Swift list III (#9), 1860 RA 02 03 33, NPD 46 04.9) is "very faint, pretty large, round". The position precesses to RA 02 12 19.8, Dec +44 34 47, just northeast of a relatively bright galaxy, so the identification is certain; the only problem is, the galaxy is the same one listed as NGC 846 (which see), so NGC 847 is a repetition of that entry. The duplication was noticed by Spitaler soon after the publication of the NGC, as is stated in the first Index Catalog.

NGC 848 (= PGC 8299)
Discovered (Dec 11, 1885) by
Ormond Stone
Also observed (Nov 1, 1886) by Lewis Swift (list V #21)
A 13th-magnitude spiral galaxy (type SBab) in Cetus (RA 02 10 17.4, Dec -10 19 14)
Per Dreyer, NGC 848 (= Swift list V, Ormond Stone list I (#49), 1860 RA 02 03 41, NPD 100 59.0) is "most extremely faint, pretty large, very difficult, star to the northeast". (Swift's paper states (for his #21) "495-7-8-9 in field", meaning GC 495, 497, 498 and 499, which are NGC 833, 835, 838 and 839; Swift's field of view being so large that the other galaxies were within his field even though lying well to the northwest.) Apparent size 1.5 by 1.0 arcmin.
DSS image of spiral galaxy NGC 848
Above, a 2.4 arcmin wide closeup of NGC 848
Below, a 12 arcmin wide region centered on the galaxy
DSS image of region near spiral galaxy NGC 848

NGC 849 (= PGC 8286)
Discovered (1886) by
Francis Leavenworth
A 14th-magnitude lenticular galaxy (type S0) in Cetus (RA 02 10 11.2, Dec -22 19 23)
Per Dreyer, NGC 849 (= Leavenworth list II (#327), 1860 RA 02 03 43, NPD 113 00.6) is "extremely faint, very small, round (? nebulosity)". The position precesses to RA 02 10 12.1, Dec -22 20 49, about an arcmin and a half south of the galaxy; but there is nothing else nearby and the description fits, so the identification is certain. Apparent size 0.5 by 0.3 arcmin.
DSS image of lenticular galaxy NGC 849
Above, a 2.4 arcmin wide closeup of NGC 849
Below, a 12 arcmin wide region centered on the galaxy
DSS image of region near lenticular galaxy NGC 849
Celestial Atlas
(NGC 750 - 799) ←     NGC Objects: NGC 800 - 849     → (NGC 850 - 899)